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19992018
most citedThe Arcminute Microkelvin Imager

246 citations · 2.1k across the 57 of their papers we have counts for

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Showing 2004 · astro-phShow all

6 papers · 2 filters

astro-ph2004★ 38 cited

Source subtraction for the extended Very Small Array and 33-GHz source count estimates

Kieran A. Cleary, Angela C. Taylor, Elizabeth Waldram +16

We describe the source subtraction strategy and observations for the extended Very Small Array, a CMB interferometer operating at 33 GHz. A total of 453 sources were monitored at 3…

astro-ph2004★ 3 cited

The 9C Survey: a deeper source count at 15 GHz

E. M. Waldram, G. G. Pooley

Foreground radio sources are a major contaminant for centimetre-wave cosmic microwave background (CMB) measurements and the 9C survey was set up as part of the observing strategy o…

astro-ph2004★ 34 cited

Very Small Array observations of the Sunyaev-Zel'dovich effect in nearby galaxy clusters

Katy Lancaster, Ricardo Genova-Santos, Nelson Falcon +10

We present VSA observations (~34GHz) on scales ~20 arcmin towards a complete, X-ray-flux-limited sample of seven clusters at redshift z<0.1. Four have significant SZ detections in…

astro-ph2004★ 95 cited

Cosmological parameter estimation using Very Small Array data out to l=1500

Rafael Rebolo, Richard A. Battye, Pedro Carreira +29

We estimate cosmological parameters using data obtained by the Very Small Array (VSA) in its extended configuration, in conjunction with a variety of other CMB data and external pr…

astro-ph2004★ 207 cited

High sensitivity measurements of the CMB power spectrum with the extended Very Small Array

Clive Dickinson, Richard A. Battye, Kieran Cleary +29

We present deep Ka-band ( GHz) observations of the CMB made with the extended Very Small Array (VSA). This configuration produces a naturally weighted synthesized FWHM…

astro-ph2004★ 19 cited

Estimating the bispectrum of the Very Small Array data

Sarah Smith, Graca Rocha, Anthony Challinor +30

We estimate the bispectrum of the Very Small Array data from the compact and extended configuration observations released in December 2002, and compare our results to those obtaine…